Massive stellar cannibals: How stellar mergers drive mass-loss in extremely massive stars
Abstract
It has been theorized that the formation of extremely massive and supermassive stars ($>10^3\ {\rm M}_\odot$) could plausibly be the outcome of stellar mergers in low metallicity ($Z1000\,\rm M_{\odot}$ with inspiraling companions of $
Fields of Study & Subjects
Pulsars and Gravitational Waves Research
Gamma-ray bursts and supernovae
Galaxies: Formation
Evolution
Phenomena
Publication details
- Journal / source
- arXiv (Cornell University)
- Publication date
- 2 February 2026
- Document type
- Preprint